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Spherically symmetric cosmological perturbations in the de Donder gauge (III)
Authors:Mark Israelit  Bernhard Rose  Heinz Dehnen
Institution:(1) Fakultät für Physik, Universität Konstanz, Konstanz, Germany;(2) Present address: Department of Physics, University of Haifa, Oranim, 36910 Tivon, Israel
Abstract:The evolution of a perfect fluid perturbation is considered in the radiation dominated period and in the dust epoch. In the investigation we make use of the general formalism developed in previous papers.It turns out that the evolution tendency is predicted by the state of the cosmic background. The radiation dominated universe does not stimulate growing processes of the perturbation, whereas the dust dominated universe causes a growing tendency of small perfect fluid formations. The results of this work are in accordance with these obtained by the present writers in a previous work.
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